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We investigate the properties of stars participating in double compact star merger events considering interacting model of stable strange quark matter. We model the matter making it compatible with the recent astrophysical observations of…

高能天体物理现象 · 物理学 2022-05-17 Anil Kumar , Vivek Baruah Thapa , Monika Sinha

The equations of state for neutron matter, strange and non-strange hadronic matter in a chiral SU(3) quark mean field model are applied in the study of slowly rotating neutron stars and hadronic stars. The radius, mass, moment of inertia,…

核理论 · 物理学 2014-11-20 Shaoyu Yin , Jiadong Zang , Ru-Keng Su

In this paper we analyze in detail the production of strangeness in proton-proton collisions in the kinematics of large transverse momenta $p_{T}$ of produced hadrons. Using the color dipole framework, we estimated the production…

高能物理 - 唯象学 · 物理学 2021-08-04 Marat Siddikov , Iván Schmidt

We investigate realistic models of compact objects, focusing on neutron and strange stars, composed by dense matter and dark energy in the form of a simple fluid or scalar field interacting with matter. For the dark energy component, we use…

广义相对论与量子宇宙学 · 物理学 2023-08-01 Artyom V. Astashenok , Sergey D. Odintsov , Vasilis K. Oikonomou

An effective chiral Lagrangian in heavy-fermion formalism whose parameters are constrained by kaon-nucleon and kaon-nuclear interactions next to the leading order in chiral expansion is used to describe kaon condensation in dense ``neutron…

高能物理 - 唯象学 · 物理学 2011-07-19 G. E. Brown , C. -H. Lee , M. Rho , V. Thorsson

Dark matter in the universe seems to be one of the most important puzzles science has to face in this moment. In this essay we point out that dark matter could be a spin-0 fundamental interaction of Nature rather than a simple particle.…

天体物理学 · 物理学 2010-12-09 T. Matos , L. A. Urena-Lopez

We calculate saturation curves for strange hadron matter using recently constructed baryon-baryon potentials which are constrained by SU(3) symmetry. All possible interaction channels within the baryon octet (consisting of $N$, $\Lambda$,…

核理论 · 物理学 2009-10-31 V. G. J. Stoks , T. -S. H. Lee

We present a mechanism that may seed compact stellar objects with stable lumps of quark matter, or {\it strangelets}, through the self-annihilation of gravitationally accreted WIMPs. We show that dark matter particles with masses above a…

宇宙学与河外天体物理 · 物理学 2015-05-30 M. A. Perez-Garcia , J. Silk , J. R. Stone

The recent observations of neutron star mergers have changed our perspective on scalar- tensor theories of gravity, favouring models where gravitational waves travel at the speed of light. In this work we consider a scalar-tensor set-up…

广义相对论与量子宇宙学 · 物理学 2018-08-15 Javier Chagoya , Gianmassimo Tasinato

In this article, we attempt to find a singularity free solution of Einstein's field equations for compact stellar objects, precisely strange (quark) stars, considering Schwarzschild metric as the exterior spacetime. To this end, we consider…

广义相对论与量子宇宙学 · 物理学 2017-10-19 Debabrata Deb , Sourav Roy Chowdhury , Saibal Ray , Farook Rahaman , B. K. Guha

Dark matter is hypothesized to interact with ordinary matter solely through gravity and may be present in compact objects such as strange quark stars. We treat strange quark stars admixed with dark matter as two-fluid systems to investigate…

高能天体物理现象 · 物理学 2025-04-22 Yida Yang , Chen Wu , Ji-Feng Yang

Strangelets (hypothetical stable lumps of strange quarkmatter) of astrophysical origin may be ultimately detected in specific cosmic ray experiments. The initial mass distribution resulting from the possible astrophysical production sites…

核理论 · 物理学 2010-03-26 Laura Paulucci , Jorge E. Horvath

The Skyrme model provides a novel unified approach to nuclear physics. In this approach, single baryon, baryonic matter and medium-modified hadron properties are treated on the same footing. Intrinsic density dependence (IDD) reflecting the…

核理论 · 物理学 2017-01-20 Yong-Liang Ma , Mannque Rho

Ever since the discovery of neutron stars it has been realized that they serve as probes of a physical regime that cannot be accessed in laboratories: strongly degenerate matter at several times nuclear saturation density. Existing nuclear…

高能天体物理现象 · 物理学 2013-12-04 M. Coleman Miller

Relativistic heavy-ion collisions lead to a final state which has a higher degree of strangeness saturation than those of elementary collisions. A systematic analysis of this phenomenon, based on the strangeness saturation factor, is made…

高能物理 - 唯象学 · 物理学 2007-05-23 J. Cleymans , B. Kampfer , P. Steinberg , S. Wheaton

We study the partial fragmentation of a strange quark star into strangelets during the process of merger of two strange quark stars. We discuss the fate of the fragments considering their possible evaporation into nucleons. We show that…

高能天体物理现象 · 物理学 2022-11-09 Niccolò Bucciantini , Alessandro Drago , Giuseppe Pagliara , Silvia Traversi , Andreas Bauswein

The neutron to mirror neutron transitions in neutron stars would possibly result in significant effects. In this work we show that collisional decoherence entails exponential relaxation in lieu of oscillations. Decoherence is a great many…

高能物理 - 唯象学 · 物理学 2026-03-13 B. O. Kerbikov

We suggest that the fluctuations of strange hadron multiplicity could be sensitive to the equation of state and microscopic structure of strongly interacting matter created at the early stage of high energy nucleus-nucleus collisions. They…

高能物理 - 唯象学 · 物理学 2009-11-10 M. I. Gorenstein , M. Gazdzicki , O. S. Zozulya

It has been revealed using microlensing that a considerable part, possibly more than half, of the dark matter in the halo of our Galaxy consists of objects with a mass spectrum ranging from 0.05 to 0.8 of the solar mass. What is the nature…

天体物理学 · 物理学 2007-05-23 A. V. Gurevich , K. P. Zybin , V. A. Sirota

We review the state of our knowledge concerning the contribution of strange quarks to various nucleon properties. In the case of the electric and magnetic form factors, the level of agreement between theory and experiment is very…

核理论 · 物理学 2022-03-02 A. W. Thomas , P. E. Shanahan , R. D. Young
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